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The gravitational potential energy at a ...

The gravitational potential energy at a body of mass `m` at a distance `r` from the centre of the earth is U. What is the weight of the body at this distance ?

A

`U`

B

`Ur`

C

`(U)/(r)`

D

`(U)/(2r)`

Text Solution

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The correct Answer is:
To find the weight of a body of mass \( m \) at a distance \( r \) from the center of the Earth, given that its gravitational potential energy at that distance is \( U \), we can follow these steps: ### Step 1: Understand Gravitational Potential Energy The gravitational potential energy \( U \) of a body at a distance \( r \) from the center of the Earth is given by the formula: \[ U = -\frac{G M m}{r} \] where: - \( G \) is the universal gravitational constant, - \( M \) is the mass of the Earth, - \( m \) is the mass of the body, - \( r \) is the distance from the center of the Earth. ### Step 2: Relate Weight to Gravitational Force The weight \( W \) of the body at that distance is the gravitational force acting on it, which can be expressed as: \[ W = \frac{G M m}{r^2} \] This formula arises from Newton's law of gravitation, where the gravitational force is inversely proportional to the square of the distance. ### Step 3: Express Weight in Terms of Potential Energy From the expression for gravitational potential energy, we can rearrange it to find the weight: 1. We know that: \[ U = -\frac{G M m}{r} \] Therefore, we can express \( G M \) in terms of \( U \): \[ G M = -\frac{U r}{m} \] 2. Substitute \( G M \) back into the weight formula: \[ W = \frac{G M m}{r^2} = \frac{-U r}{m} \cdot \frac{m}{r^2} \] Simplifying this gives: \[ W = -\frac{U}{r} \] ### Step 4: Final Expression for Weight Thus, the weight of the body at a distance \( r \) from the center of the Earth can be expressed as: \[ W = -\frac{U}{r} \] ### Conclusion The weight of the body at a distance \( r \) from the center of the Earth, given its gravitational potential energy \( U \), is: \[ W = -\frac{U}{r} \]

To find the weight of a body of mass \( m \) at a distance \( r \) from the center of the Earth, given that its gravitational potential energy at that distance is \( U \), we can follow these steps: ### Step 1: Understand Gravitational Potential Energy The gravitational potential energy \( U \) of a body at a distance \( r \) from the center of the Earth is given by the formula: \[ U = -\frac{G M m}{r} \] where: ...
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